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Change of primary cosmic ray mass composition at superhigh energies
Authors:N N Kalmykov  Jorge Cotzomi  V P Sulakov  Yu A Fomin
Institution:(1) Institute of Nuclear Physics of Moscow State University, Moscow, Russia;(2) Chair of Cosmic Physics, Moscow State University, Moscow, Russia
Abstract:The EAS MSU array experimental data are analyzed in relation to the primary cosmic ray composition in the energy range above 1017–1018 eV. The problem of the existence of an additional cosmic ray component, which cannot be explained in the framework of traditional mechanism of Galactic cosmic ray production, is considered. The fraction of gamma-quanta in the primary cosmic radiation is evaluated as well.
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